An algorithm for the synthesis of binary sequence detectors
Algorithm for synthesis of binary sequence detectors
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Algorithm for synthesis of binary sequence detectors
Rotating emission ring in terms of stability of periodic orbits in restricted three-body problem for binary systems
Channel error effect on sample compression system employing binary sequence time encoding
Crystallization kinetics of molten binary and ternary oxide systems
Thermodynamic analysis of binary vapor liquid equilibria
Theoretical investigation of atmosphere of binary stars based on analogy between gas dynamics and shallow water flow
Chernoff bound and tilted distribution argument for obtaining error probability bounds for binary signaling on slowly fading Rician channel
Contact binaries origin and evolution, discussing orbital angular momentum dissipation through mass ejection along magnetic lines of force
Age and helium content correlations from recent mass determinations of two low mass binary star systems used in stellar evolution theory
Representation of rotating gaseous emission rings in eclipsing binary systems by periodic orbits around more massive component in restricted three-body problem
Mass transfer cooling of carbon dioxide-nitrogen binary system in laminar boundary layer, stressing dissociation effect
We present the discovery of two T dwarf binaries, 2MASS 1225-2739AB and 2MASS 1534-2952AB, identified in a sample of ten T dwarfs imaged with the Huble Space Telescope Wide Field Planetary Camera 2.
We present new emission line spectra and an analysis of the mass outflow for the massive binary, HD 149404.
An Investigation of the statistical description of binary mixing and/or reaction between a carrier gas and an evaporated vapor species in two-phase gas-liquid turbulent flows is perfomed through both theroetical analysis and comparisons with results from direct numerical simulations (DNS) of a two-phase mixing layer.
A method has been developed to improve on Witten's binary arithmetic coding procedure of tracking a high value and a low value. The new method approximates the probability of the less probable symbol, which improves the worst-case coding efficiency.
Evaporation and ignition of a binary-fuel cluster of drops is described by models under the.
Hubble Space Telescope images of HK Tauri reveal that the companion star in this 2.4 in (340 AU) pre-main sequence binary system is an entirely nebulous object at visual wavelengths.
We report on Chandra X-ray Observatory (Chandra) High Energy Transmission Grating spectra of the dipping low-mass X-ray binary 1A 1744−361 during its 2008 July outburst. We find that its persistent emission is well modeled by a blackbody (kT approx. 1.0 keV) plus power law (Gamma approx. 1.7) with an absorption edge. In the residuals of the combined spectrum, we find a significant absorption line at 6.961 +/- 0.002 keV, consistent with the Fe xxvi (hydrogen-like Fe) 2-1 transition.We place an upper limit on the velocity of a redshifted flow of nu < 221 km/s. We find an equivalent width for the line of 27+2/−3 eV, from which we determine a column density of (7 +/- 1)×10(exp 17) /sq. cm via a curve-of-growth analysis. Using XSTAR simulations, we place a lower limit on the ionization parameter of >103.6 erg cm/s. We discuss what implications the feature has on the system and its geometry. We also present Rossi X-ray Timing Explorer data accumulated during this latest outburst and, via an updated color-color diagram, clearly show that 1A 1744−361 is an "atoll" source